Exploring Early Galaxies: James Webb Space Telescope Challenges Gravity Theories

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15/11/2024 20h40

**James Webb Space Telescope Observations Challenge Established Gravity Theories**

Astronomers utilizing the James Webb Space Telescope (JWST) to explore the distant past of the universe have uncovered findings that may support an alternative theory of gravity. A team from Case Western Reserve University claims that the images of early galaxies captured by JWST contradict the predictions made by the widely accepted Lambda Cold Dark Matter (Lambda-CDM) theory, suggesting instead a basis for a theory known as Modified Newtonian Dynamics (MOND).

The Lambda-CDM model has long maintained that dark matter, an invisible and mysterious form of matter, plays a crucial role in galaxy formation. According to this theory, dark matter's gravitational pull should cause ancient galaxies in the early universe to appear small and dim as they gradually cluster together over time. However, the team led by Stacy McGaugh has observed that these galaxies instead appear bright, large, and fully formed, challenging the conventional understanding of galaxy formation driven by dark matter.

"Dark matter was hypothesized to explain how we moved from a uniform early universe to the large, complex galaxies with significant empty spaces that we see today," McGaugh, a professor and the director of astronomy at Case Western Reserve, stated. "But our observations do not align with the predictions made by the dark matter theory."

MOND, first proposed in 1983 by physicist Mordehai Milgrom, offers a different perspective. It suggests slight modifications to Newton's second law in regions of very small accelerations, like those at the universe's edges. According to MOND, galaxies could have formed quickly without the need for dark matter. McGaugh, along with his colleagues who co-authored a significant paper in 1998, theorized that galactic material was swiftly collected and expanded with the universe before collapsing under its own gravity to form galaxies.

The recent data from JWST appear to support MOND predictions more closely than those of Lambda-CDM. For instance, MOND-based predictions by R H Sanders have shown a better match with the observational data than the predictions made by Lambda-CDM proponents like Mo, Mao, and White. Despite these findings, MOND remains controversial due to difficulties in reconciling it with Einstein's Theory of General Relativity.

While MOND has gained some traction from the recent JWST observations, the Lambda-CDM model continues to be widely supported within the scientific community. Since its inception in the 1920s, Lambda-CDM has accurately described the universe's expansion and provided a coherent framework for understanding cosmology. Nonetheless, McGaugh welcomes the debate prompted by these new discoveries.

"The expectation was that large galaxies in the nearby universe would have formed from small pieces over time, but that's not what JWST is showing us," McGaugh remarked. Although finding a theory that harmonizes both General Relativity and MOND remains an unresolved challenge, McGaugh feels somewhat vindicated by the recent findings. "The bottom line is, 'I told you so,'" he noted, emphasizing the importance of making predictions and testing their validity as a fundamental aspect of the scientific method.

This groundbreaking research, entitled "Accelerated Structure Formation: The Early Emergence of Massive Galaxies and Clusters of Galaxies," was published in The Astrophysical Journal on November 12, 2024.

The views expressed in this article do not reflect the opinion of ICARO, or any of its affiliates.

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